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From the 1 of 7 linked papers with an AI index.

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7 papers

astro-ph.GA2026

A differentiable hydrodynamical approach to the Milky Way bar pattern speed with CO longitude--velocity data

Junichi Baba, Kohei Hattori

The paper presents a differentiable hydrodynamical framework that simulates gas flow in the Milky Way’s barred potential and uses CO longitude‑velocity data to constrain the bar’s…

astro-ph.GA2026

Axisymmetric Jeans modelling systematically overestimates the circular speed in the inner Milky Way

Tomoki Yamaguchi, Junichi Baba

We quantify systematic biases in rotation curves inferred from steady, axisymmetric Jeans modelling when the underlying stellar velocity field is non-axisymmetric. Using a high-res…

astro-ph.GA2026

Vaulting the barrier: An intrinsic mechanism to fuel the gas beyond the nuclear ring into the central region of barred galaxies

Kotaro Kobayashi, Naomichi Yutani, Takayuki R. Saitoh +2

Gas delivery to galactic centers powers nuclear starbursts and active galactic nuclei (AGNs), yet bar-driven inflow is generally expected to stall in a nuclear ring a few hundred p…

astro-ph.GA2026

Bar-Informed Kinematic-Distance Mapping of Molecular Gas in the Inner Milky Way

Junichi Baba

We present a bar-informed kinematic-distance (BIKD) method to reconstruct face-on molecular-gas maps of the inner Milky Way from PPV data, relaxing the standard assumption of axisy…

astro-ph.GA2026

Kinematic-Distance Biases in the Inner Milky Way from a Stellar-Dynamically Constrained Bar

Junichi Baba

We quantify how bar-driven non-circular motions bias Milky-Way gas maps inferred with the kinematic-distance (KD) method. KD reconstructions of H\,\textsc{i} and CO surveys assume…

astro-ph.GA2025

Bar-driven Streaming Motions Mimic a Massive Bulge in the Inner Milky Way

Junichi Baba

The circular speed curve of the Milky Way provides a key constraint on its mass distribution, reflecting the axisymmetric component of the gravitational potential. This is especial…